中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Chemical models of interstellar glycine and adenine precursor aminoacetonitrile (NH2CH2CN)

文献类型:期刊论文

作者Zhang, Xia4,5; Quan, Donghui1,4; Li, Xiaohu2,4,5; Esimbek, Jarken2,4,5; Li, Fangfang4; Zhou, Yan3; Li, Dalei2,4,5
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2024-09-04
卷号533期号:3页码:3623-3636
关键词astrochemistry molecular processes ISM: abundances ISM: molecules
ISSN号0035-8711
DOI10.1093/mnras/stae2000
产权排序1
英文摘要Aminoacetonitrile (AAN), also known as glycinenitrile, has been suggested as a possible precursor of glycine and adenine in the interstellar medium. Here we present the chemical modeling of AAN and its isomers in hot cores using the three-phase chemical model NAUTILUS with the addition of over 300 chemical reactions of the three AAN isomers and related species. Our models predicted a peak gas phase abundance of AAN reaching the order of 10(-8), which is consistent with observation towards Sgr B2(N). Regarding the reaction pathways of AAN and its isomers, we found that AAN is primarily formed via free radical reactions on grain surfaces during the early evolutionary stages. Subsequently, it is thermally desorbed into the gas phase as the temperature rises and is then destroyed by positive ions and radicals in gas phase. The isomers of AAN are formed through the hydrogenation reaction of CH3NCN on the grain surface and via electron recombination reactions of ion C2H5N2+ in gas phase. We speculate that there is a possibility for NCCN and AAN to react with each other, eventually leading to the formation of adenine in hot cores. However, further investigation is required to understand the efficiency of grain surfaces in adenine formation, through theoretical calculations or laboratory experiments in future research
WOS关键词EXPLORING MOLECULAR COMPLEXITY ; COUPLED-CLUSTER SINGLES ; HOT CORES ; ORGANIC-MOLECULES ; AMINO-ACIDS ; CHEMISTRY ; GAS ; PHASE ; ENERGY ; HYDROGENATION
资助项目National Natural Science Foundation of China[12203091] ; National Natural Science Foundation of China[12373026] ; National Natural Science Foundation of China[12173075] ; National Natural Science Foundation of China[2022D01A156] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[2022YFA1603103] ; National Key R&D Program of China ; Youth Innovation Promotion Association CAS
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001305885900011
出版者OXFORD UNIV PRESS
资助机构National Natural Science Foundation of China ; National Natural Science Foundation of China ; Natural Science Foundation of Xinjiang Uygur Autonomous Region ; National Key R&D Program of China ; Youth Innovation Promotion Association CAS
源URL[http://ir.xao.ac.cn/handle/45760611-7/6972]  
专题天体化学研究团组
通讯作者Zhang, Xia; Quan, Donghui; Li, Xiaohu
作者单位1.Zhejiang Lab, Res Ctr Astron Comp, Hangzhou 311100, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China
3.Shandong Univ Aeronaut & Astronaut, Coll Sci, 391 Huanghe 5th Rd, Binzhou City 256600, Shandong, Peoples R China
4.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
5.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Peoples R China
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GB/T 7714
Zhang, Xia,Quan, Donghui,Li, Xiaohu,et al. Chemical models of interstellar glycine and adenine precursor aminoacetonitrile (NH2CH2CN)[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,533(3):3623-3636.
APA Zhang, Xia.,Quan, Donghui.,Li, Xiaohu.,Esimbek, Jarken.,Li, Fangfang.,...&Li, Dalei.(2024).Chemical models of interstellar glycine and adenine precursor aminoacetonitrile (NH2CH2CN).MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,533(3),3623-3636.
MLA Zhang, Xia,et al."Chemical models of interstellar glycine and adenine precursor aminoacetonitrile (NH2CH2CN)".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 533.3(2024):3623-3636.

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